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ESO 140-43

Observation

Spectrum ID478399456_sp2
Alt nameg1844540-622153
z0.0139
RA, Dec281.2249, -62.3647
MJD59500.38
SNR/Å B/R9.8/21.9
Obs Airmass1.23
SMSS ID478399456
Closest SMSSNone (< 15")
SMSS Mean r6"ap14.4 ± 0.1
2MASS Kext9.7 ± 0.0

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.093
Power law αν-1.64 ± 0.19
log L5100,AGN42.94 ± 0.02
log HβBr/[O III]-0.04 ± 0.04
log ML5100/M7.35 ± 0.09
log M/M7.03 ± 0.04
log M/M7.31 ± 0.10
log M[O III]/M7.47 ± 0.09

Spatial extraction & sky subtraction region

Spatial plot

Spaxel scale: 1 arcsec² — Flux units: erg s⁻¹ cm⁻² Å⁻¹
Apertures: object (solid), background (dashed)

Spectrum decomposition

Emission line measurements

Linelog L (erg s⁻¹)FWHM (km s⁻¹)σ (km s⁻¹)EW (Å)
Hγ Narrow39.58 ± 0.19287 ± 63208 ± 392.05 ± 0.61
Hγ Broad40.40 ± 0.101639 ± 480598 ± 17312.43 ± 0.93
[O III] 436439.41 ± 0.18264 ± 63111 ± 251.44 ± 0.35
He II Narrow39.43 ± 0.17264 ± 63111 ± 251.53 ± 0.29
He II Broad40.26 ± 0.281854 ± 1677787 ± 7128.33 ± 0.77
Hβ Narrow40.07 ± 0.08287 ± 63208 ± 396.76 ± 0.49
Hβ Broad41.07 ± 0.042825 ± 2681151 ± 19868.87 ± 1.03
[O III] 500741.11 ± 0.01287 ± 63208 ± 3974.83 ± 0.50
He I Narrow39.06 ± 0.18264 ± 63111 ± 250.70 ± 0.16
He I Broad40.32 ± 0.062763 ± 4171173 ± 17712.65 ± 0.56
[O I] 630039.52 ± 0.06264 ± 63111 ± 252.13 ± 0.16
Hα Narrow40.63 ± 0.01264 ± 63111 ± 2527.40 ± 0.25
Hα Broad41.75 ± 0.012163 ± 871083 ± 31356.36 ± 0.73
[N II] 658540.55 ± 0.02264 ± 63111 ± 2522.41 ± 0.22
[S II] 671840.07 ± 0.02264 ± 63111 ± 257.64 ± 0.18
[S II] 673240.04 ± 0.02264 ± 63111 ± 257.15 ± 0.18

All narrow line widths are tied to narrow [O III] 5007Å. [O III] 5007Å and narrow Hβ include a second narrow component not tied to other narrow lines.

Emission summary

Hα Broad SNR38.10
Hβ Broad SNR9.38
Hγ Broad SNR3.71
AGN frac0.76
Host frac0.23
log L5100,Host42.43
Fe II/Hβ0.36
Fe II/[O III]0.34

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width0
balmer_width0

Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.